Determining the orbital period of a satellite requires knowledge of its radius, as per Kepler's Law, and cannot be calculated with only the gravitational constant (G) and Earth's mass. The relationship established by Kepler indicates that the square of the orbital period is proportional to the cube of the radius. When calculating Earth's mass using the moon's orbit, it is suggested to subtract the moon's mass from the total to achieve a more accurate result. The calculation provided shows that after accounting for the moon's mass, Earth's mass is approximately 5.99E+24 kg. Accurate calculations are essential for precise astrophysical measurements.